Galaxy clusters seen in X-rays: from the most relaxed to the most perturbed

Details Galaxy clusters seen in X-rays: from the most relaxed to the most perturbed Galaxy clusters seen in X-rays: from the most relaxed to the most perturbed

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005sf2a.conf..709d&link_type=abstract

SF2A-2005: Semaine de l'Astrophysique Francaise, meeting held in Strasbourg, France, June 27 - July 1, 2005, Edited by F. Casoli

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

We present recent X-rays, optical and radio observations of the rich clusters of galaxies Abell 85, 496, 2667, and 3376. Detailed analysis of these clusters shows that none of them is strictly relaxed, all of them revealing to some degree signs of recent dynamical activity. We show how temperature maps and multi-wavelength observations are powerful tools to probe the history of galaxy clusters. %

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